Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2003, Vol. 27> Issue(11) : 978-983 

Abundance Distribution in the Solar System and Slow Neutron Capture Elements in AGB Stars

  •  Academy of Physics and Information Engineering, Guangxi Normal University, Guilin 541004, China2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039, China3 Department of Physics, Hehei Normal University, Shijiazhuang 050016, China4 Center of Theoretical Nuclear Physics, National laboratory of Heavy Ion Accelerator of Lanzhou, I-an/.hou 730000, China

  • By re-analyzing the results of the theoretical abundance of AGB stellar models and the observed abundances of 51 AGB samples, we find that the abundance distribution of heavy elements belonging to the main-component of slow neutron capture process (SMH elements) of any AGB star is similar to that of the scaled s-process main component of the solar system. It means that superposition of the SMH element abundance distributions of AGB stars should be similar to that of the scaled solar s-main component. As a conclusion, the heavy element abundance pattern of the solar s-main component is a typical one and can be used as a standard in the investigation of heavy element abundances in single star.
  • 加载中

  • References

    [1] Burbidge E M, Berbidge G R, Fowler W A et al. Rev. Mod. Phys., 1957,29: 547–6502 ZHANG Miao–Jing, ZHANG Bo, LI Guang–Lie. Nucl. Phys. Rev., 2002,19:321–328(in Chinese)(张妙静,张波,厉光烈.原子核物理评论,2002,19:321–328)3 Wallerstein G, Greenstein J L, Parker R et al. Ap. J., 1963,137:280–3004 Spite M, Spite F. Astron, Astrophys., 1978,67:23–315 Woolf V M, Tomkin J, Lambert D L. Ap. J., 1995,453:660–6726 Gallino R, Arlandini C, Busso M et al. Ap. J., 1998,497:388–4037 Travaglio C, Galli D, Gallino R et al. Ap. J., 1999,521:691–7028 Busso M, Gallino R,Lambert D Let al. Ap. J., 2001,557:802–8219 Arlandini C, Kppeler F, Wisshak K et al. Ap. J., 1999,525:886–90010 Luck R E, Bond H E. Ap. J., 1985, 292:559–57711 Luck R E, Bond H E. Ap. J. Suppl., 1991,77:515–54012 Abia C, Wallerstein G. Mon. Not. R. Astron. Soc., 1998,293:89–10613 Abia C, Isern J. Ap. J., 2000,536:438–449 14 Abia C, Dominguez I, Gallino R et al. Ap. J., 2002,579:817–83115 Van Eck S, Goriely S, Jorissen A et al. Nature, 2001,412:793–79516 Aoki Wako, Ryan S G, Norris J E et al. Ap. J., 2001,561:346–36317 ZHANG Miao–Jing et al. High Energy Phys. and Nucl. Phys., 2003, 27(4) :304–308(in Chinese)(张妙静等.高能物理与核物理,2003,27(4) :304–308)

  • Access

    加载中

Get Citation
ZHANG Miao-Jing, ZHANG Bo and LI Guang-Lie. Abundance Distribution in the Solar System and Slow Neutron Capture Elements in AGB Stars[J]. Chinese Physics C, 2003, 27(11): 978-983.
ZHANG Miao-Jing, ZHANG Bo and LI Guang-Lie. Abundance Distribution in the Solar System and Slow Neutron Capture Elements in AGB Stars[J]. Chinese Physics C, 2003, 27(11): 978-983. shu
Milestone
Received: 2003-04-29
Revised: 1900-01-01
Article Metric

Article Views(2549)
PDF Downloads(572)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Abundance Distribution in the Solar System and Slow Neutron Capture Elements in AGB Stars

    Corresponding author: ZHANG Miao-Jing,
  • Academy of Physics and Information Engineering, Guangxi Normal University, Guilin 541004, China2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039, China3 Department of Physics, Hehei Normal University, Shijiazhuang 050016, China4 Center of Theoretical Nuclear Physics, National laboratory of Heavy Ion Accelerator of Lanzhou, I-an/.hou 730000, China
  • Received Date: 2003-04-29
  • Accepted Date: 1900-01-01
  • Available Online: 2003-11-05

Abstract: By re-analyzing the results of the theoretical abundance of AGB stellar models and the observed abundances of 51 AGB samples, we find that the abundance distribution of heavy elements belonging to the main-component of slow neutron capture process (SMH elements) of any AGB star is similar to that of the scaled s-process main component of the solar system. It means that superposition of the SMH element abundance distributions of AGB stars should be similar to that of the scaled solar s-main component. As a conclusion, the heavy element abundance pattern of the solar s-main component is a typical one and can be used as a standard in the investigation of heavy element abundances in single star.

    HTML

Reference (1)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return